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One of the primary sources for the future space-based gravitational wave detector, the Laser Interferometer Space Antenna, are the inspirals of small compact objects into massive black holes in the centres of galaxies.
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Rapid generation of fully relativistic extreme-mass-ratio-inspiral waveform templates for LISA data analysis
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Constraining the spin parameter of near-extremal black holes using lisa
O. Burke, J. R. Gair, J. Simón, and M. C. Edwards · 2020
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Gravitational wave cosmology with extreme mass-ratio inspirals, 2021
D. Laghi et al · 2021
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Formation rate of extreme mass ratio inspirals in active galactic nucleus, 2021
Z. Pan and H. Yang · 2021
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FastEMRIWaveforms: New tools for millihertz gravitational-wave data analysis
M. L. Katz et al · 2021
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Non-linear effects in emri dynamics and their imprints on gravitational waves, 2021
G. Lukes-Gerakopoulos and V. Witzany · 2021
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